Who's in the Driver's Seat: Magnetic Fields or Turbulence?

Details Who's in the Driver's Seat: Magnetic Fields or Turbulence? Who's in the Driver's Seat: Magnetic Fields or Turbulence?

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jrasc..99r.143p&link_type=abstract

Journal of the Royal Astronomical Society of Canada, Vol. 99, No. 4, p.143

Astronomy and Astrophysics

Astronomy

Scientific paper

New polarization data at 850 microns of OMC2 in Orion A are presented. These measurements trace the direction of magnetic fields in the densest parts of the filamentary molecular clouds and form a part of the comparison of magnetic-field directions at various spatial and density scales. They allow us to put constraints on existing models, and better understand the competitive role of magnetic fields and turbulence in the ISM and in the process of star formation.

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